NAWDIC

North Atlantic Waveguide, Dry Intrusion, and Downstream Impact Campaign
Mission status: Scheduled
Persons in Charge
Mission-PI
Julian Quinting, Annika Oertel (KIT), Andreas Schäfler (DLR)
Mission coordinator
Bastian Kirsch (KIT)
Contact point at DLR-FX for this mission:
Address
HALO Deployment Base
Time Period
October 2025 – February 2026
Mission phase | Dates |
---|---|
Preparation, Payload Integration, EMI Testing | 27 Oct - 19 Dec 2025 |
Mission Execution | 13 Jan - 20 Feb 2026 |
Dismounting of Payload | 23 Feb - 27 Feb 2026 |
Project description
In boreal winter, gale-force wind gusts, widespread heavy precipitation, and cold-air outbreaks constitute some of the most severe weather hazards affecting Europe. Advancing our understanding of the synoptic- to micro-scale processes and their representation in numerical weather prediction (NWP) models leading to such hazardous high impact weather (HIW) is the overarching aim of the ground-based and airborne “North Atlantic Waveguide, Dry Intrusion, and Downstream Impact Campaign” (NAWDIC, https://www.nawdic.kit.edu/). The core element of the international NAWDIC consortium is NAWDIC-HALO. The NAWDIC-HALO consortium comprises German institutions working on topics of mid-latitude atmospheric dynamics. It is led by the Institute of Meteorology and Climate Research, Troposphere Research (IMKTRO) of the Karlsruhe Institute of Technology (KIT), and further consists of the University of Mainz, Ludwig-Maximilians-University of Munich and DLR’s (German Aerospace Center) Institute of Atmospheric Physics. At an international level, NAWDIC has matured into a large pan-Atlantic consortium with scientific partners from 10 countries involving universities, research institutions and weather services. NAWDIC is endorsed by WMO’s World Weather Research Programme (WWRP).
Despite significant advancements of state-of-the-art NWP models in recent decades, accurately forecasting the location, timing, and intensity of mesoscale HIW events remains a challenge. This is to a large degree due to the cross-scale interactions of physical processes involved in the formation of HIW. In midlatitudes, the processes range from upper-tropospheric Rossby waves covering thousands of kilometers and lasting several days to turbulent momentum transport in the planetary boundary layer (PBL) and cloud microphysical processes acting on scales of hundreds of meters to micrometers and minutes to seconds. A cross-scale airstream that connects upper-tropospheric Rossby waves over North America and the Atlantic Ocean with HIW in Europe is the dry intrusion (DI). During winter months, DIs emerge most frequently from the downstream flank of upper-tropospheric ridges over eastern North America. From this region (referred to as ‘DI inflow’), the DI descends equatorward into the cold sector of a downstream extratropical cyclone over a horizontal distance of 1000-5000 km and reaches the PBL about 2 days later (referred to as ‘DI outflow’). The DI outflow is accompanied by intense surface heat and moisture fluxes, elevated PBL heights, changes in PBL cloud cover, and a destabilization of the lower troposphere leading to unusually strong wind gusts and extreme rainfall due to deep convection. Most of the time, the involved cross-scale interactions of physical processes relevant to HIW in Europe occur upstream over the Atlantic Ocean and are insufficiently captured by operational observing systems.

Accordingly, modern measurement systems on research aircraft are the only way to obtain reliable observations with the necessary high spatial and temporal resolution in these remote regions. With its long range and advanced instrumentation, HALO is optimal to characterize the structure of the DI inflow and outflow, and thus to bridge the scales from the upper-tropospheric Rossby wave to HIW in the PBL. This requires multiple consecutive flights on different days and in two regions of the DI airstream:
- Two to three days before a forecasted HIW event, HALO will sample the structure of the upper troposphere and lower stratosphere in the DI inflow region, which affects the evolution of the DI itself and the downstream development.
- Closer to the event, HALO will document mesoscale processes at the DI outflow–PBL and DI outflow–cold front interfaces which are directly linked to HIW and precondition the atmosphere for subsequent cyclone development.
A tailored payload combining remote sensing and dropsonde observations will allow us to sample these regions at unprecedented detail and precision, which is necessary for a targeted evaluation of the quality of operational observing and analysis systems in regions crucial for HIW.
Partners
- Karlsruhe Institute of Technology (KIT)
- Institute for Atmospheric Physics, German Aerospace Center (DLR-IPA)
- Johannes Gutenberg Universität Mainz (JGU)
- Ludwig-Maximilians-Universität Munich (LMU)
- Forschungszentrum Jülich (FZJ)
Scientific instruments and payload configuration
List of scientific instruments for the mission:
Scientific instrument acronym | Description | Principal investigator | Institution |
---|---|---|---|
WALES | four-wavelength differential absorption lidar | Martin Wirth | DLR-IPA |
HEDWIG | Heterodyne Detection WIndlidar Gadget | Benjamin Witschas | DLR-IPA |
KITsonde | modular multi-sensor dropsonde system | Andreas Wieser | KIT |
specMACS | imaging cloud spectrometer for the solar spectral range | Tobias Zinner | LMU Munich |
UMAQS | Quantum cascade laser absorption spectroscopy | Peter Hoor | JGU Mainz |
FISH | Fast In-situ Stratospheric Hygrometer | Christian Rolf | FZ Jülich |
FAIRO | Ozone detector | Andreas Zahn | KIT |
BAHAMAS | HALO Basic Data Acquisition System | Andreas Giez | DLR-FX |
Cabin and exterior configuration of HALO for the mission
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HALO flights for this mission
Aircraft registration | Date | Take off - Landing / UT | Total flight time / h | From - To | Mission # |
---|---|---|---|---|---|
D-ADLR | yyyy-mm-dd | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 1 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 2 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 3 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 4 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 5 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 6 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 7 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 8 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 9 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 10 |
D-ADLR | Date | hh:mm:ss - hh:mm:ss | h | CODE - CODE | 11 |